Contribution of nuclei accelerated by gamma-ray pulsars to cosmic rays in the Galaxy
- 28 February 2002
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 16 (4) , 397-409
- https://doi.org/10.1016/s0927-6505(01)00124-4
Abstract
No abstract availableKeywords
All Related Versions
This publication has 39 references indexed in Scilit:
- A measurement of the cosmic ray spectrum and composition at the kneeAstroparticle Physics, 2001
- Ultra–High-Energy Cosmic Rays from Young Neutron Star WindsThe Astrophysical Journal, 2000
- The cosmic ray composition between 1014 and 1016 eVAstroparticle Physics, 1999
- Gamma-rays and neutrinos from very young supernova remnantsAstroparticle Physics, 1998
- High energy cosmic ray spectroscopy. III. Further analysesAstroparticle Physics, 1998
- Gamma Rays and Neutrinos from the Crab Nebula Produced by Pulsar Accelerated NucleiPhysical Review Letters, 1997
- Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high energiesPhysical Review Letters, 1993
- Energetic radiation from rapidly spinning pulsars. I - Outer magnetosphere gaps. II - VELA and CrabThe Astrophysical Journal, 1986
- Origin of energetic cosmic rays. II. The possibility of a contribution from pulsarsJournal of Physics A: Mathematical, Nuclear and General, 1974
- On the Nature of Pulsars. I. TheoryThe Astrophysical Journal, 1969